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Exceeding the leading spike intensity and fluence limits in backward Raman amplifiers
V M Malkin1, Z Toroker2, N J Fisch1
1Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08540, USA.
Abstract:
The leading amplified spike in backward Raman amplifiers can reach nearly relativistic intensities before the saturation by the relativistic electron nonlinearity. The saturation sets an upper limit to the largest achievable leading spike intensity. It is shown here that this limit can be substantially exceeded by the initially subdominant spikes, which surprisingly outgrow the leading spike after its nonlinear saturation. Furthermore, an initially negligible group velocity dispersion of the amplified pulse in strongly undercritical plasma appears to be capable of delaying the longitudinal filamentation instability in the nonlinear saturation regime. This enables further amplification of the pulse to even larger output fluences.
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